14 papers found
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Planck Far-infrared Detection of Hyper Suprime-Cam Protoclusters at z ∼ 4: Hidden AGN and Star Formation Activity
Planck far-infrared detection of Hyper Suprime-Cam protoclusters at $\bf z∼4$: hidden AGN and star formation activity
SILVERRUSH. VII. Subaru/HSC Identifications of Protocluster Candidates at z ∼ 6–7: Implications for Cosmic Reionization
SILVERRUSH. VII. Subaru/HSC Identifications of 42 Protocluster Candidates at z~6-7 with the Spectroscopic Redshifts up to z=6.574: Implications for Cosmic Reionization
Luminous quasars do not live in the most overdense regions of galaxies at z ∼ 4
Galaxy Protoclusters as Drivers of Cosmic Star Formation History in the First 2 Gyr
Cosmic Galaxy-IGM H i Relation atz∼ 2–3 Probed in the COSMOS/UltraVISTA 1.6 Deg2Field
Cosmic Galaxy-IGM H i Relation at z~ 2--3 Probed in the COSMOS/UltraVISTA 1.6 Deg2 Field
LARGE-SCALE STRUCTURE AROUND Az= 2.1 CLUSTER
HSTEMISSION LINE GALAXIES ATz∼ 2: COMPARING PHYSICAL PROPERTIES OF LYMAN ALPHA AND OPTICAL EMISSION LINE SELECTED GALAXIES
SURVEYING GALAXY PROTO-CLUSTERS IN EMISSION: A LARGE-SCALE STRUCTURE ATz= 2.44 AND THE OUTLOOK FOR HETDEX
DISCOVERY OF a LARGE NUMBER OF CANDIDATE PROTOCLUSTERS TRACED BY ∼15 Mpc-Scale GALAXY OVERDENSITIES IN COSMOS
Ancient Light From Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters
The long-term variability of the X-ray sources in M82
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